PSF fitting photometry of the [O i], r′, and H _α images in Figure 3 of θ ¹ Ori C ₁ C ₂ with a 44% Strehl theoretical PSF gave a good fit to both binary components in all cases. For 2012 December 12 UT we find separation is 32.64 ± 0.48 mas and PA is 206 31 ± 0 17. Here we plot this position (in red) against the interferometric orbit of Kraus et al. (2009). The agreement with the predicted position of C ₂ w.r.t. C ₁ is reasonable given the uncertainty of the orbital solution. However, more VisAO astrometry at this level of accuracy following this poorly sampled side (20° < PA < 210°) of the orbit over the next few years would certainly lead to a better orbital solution than is known today.